Photometric study of the open cluster NGC 2323

被引:20
作者
Claria, JJ [1 ]
Piatti, AE [1 ]
Lapasset, E [1 ]
机构
[1] Univ Nacl Cordoba, Astron Observ, RA-5000 Cordoba, Argentina
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1998年 / 128卷 / 01期
关键词
open clusters; individual; NGC; 2323; general; HR diagram;
D O I
10.1051/aas:1998130
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
UBV photoelectric photometry for 175 stars in the field of the southern open cluster NGC 2323, supplemented by DDO photometry of 5 probable giants, is presented. The analysis of the photometric data yields 109 probable members; one of them being a red giant, and 3 possible members. The reddening across the cluster is slightly variable and the mean value E(B - V) = 0.25. The apparent cluster distance modulus is 10.62, corresponding to a distance of 940 pc. The age, determined by fitting isochrones with core overshooting, turns out to be 100 +/- 20 Myr. Other fundamental cluster parameters are also determined. NGC 2323 appears not to be physically connected to the CMa OB1 association.
引用
收藏
页码:131 / 138
页数:8
相关论文
共 37 条
[1]  
[Anonymous], 1953, Statistical astronomy
[2]   SELF-CONSISTENT DETERMINATIONS OF THE TOTAL AMOUNT OF MATTER NEAR THE SUN [J].
BAHCALL, JN .
ASTROPHYSICAL JOURNAL, 1984, 276 (01) :169-181
[3]   POSSIBILITY OF MASS LOSS IN RED-GIANT STAGE FROM H-R DIAGRAMS OF GALACTIC CLUSTERS [J].
BARBARO, G ;
DALLAPORTA, N ;
FABRIS, G .
ASTROPHYSICS AND SPACE SCIENCE, 1969, 3 (01) :123-+
[4]  
BARKHATOVA KA, 1950, ASTRON ZH, V27, P182
[5]  
Becker W., 1971, ASTRON ASTROPHYS S, V4, P241
[6]  
BERTELLI G, 1994, ASTRON ASTROPHYS SUP, V106, P275
[7]  
BURKI G, 1975, ASTRON ASTROPHYS, V43, P37
[8]  
CAILLAULT JP, 1994, AIP C P, V313, P7
[9]  
Claria J. J., 1973, Astronomy and Astrophysics Supplement Series, V9, P251
[10]   MEMBERSHIP, FUNDAMENTAL PARAMETERS AND LUMINOSITY FUNCTION OF THE OPEN CLUSTER NGC-5662 [J].
CLARIA, JJ ;
LAPASSET, E ;
BOSIO, MA .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1991, 249 (02) :193-207